A Study of the Background in the HETE Equatorial Orbit
著者
和文:
Butler, N.,
Dullighan, A.,
Atteia, J.-L.,
河合 誠之,
Yoshida, A.,
Tamagawa, T. ..
英文:
Butler, N.,
Dullighan, A.,
Atteia, J.-L.,
Kawai, N.,
Yoshida, A.,
Tamagawa, T. ..
言語
English
掲載誌/書名
和文:
英文:
Gamma-Ray Burst and Afterglow Astronomy 2001: A Workshop Celebrating the First Year of the HETE Mission
巻, 号, ページ
Vol. 662
pp. 63-65
出版年月
2003年4月
出版者
和文:
英文:
会議名称
和文:
英文:
開催地
和文:
英文:
アブストラクト
After a year of operation, we have become well acquainted with HETE's in-orbit background. In particular, as it is near solar maximum, we have observed through intense periods of geomagnetic disturbance. We describe the resulting deviations from our mean backgrounds. Aside from these periods, the background has been quite stable over this first year. We compare the averaged background in the WXM and Fregate instruments for the months of March and September, 2001.
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